English (United Kingdom)

https://curated-unify.zendy.io/wp-json/zendy-region/v1/featured_content/oa?rat=en

https://curated-unify.zendy.io/wp-json/zendy-region/v1/highlighted_journal/

Global: Zendy Plus annual

Presents the access of premium content as premium feature

Premium Content

Presents the keyphrase highlighting as premium feature

Keyphrase Highlighting

Presents the summarisation as premium feature

Summarisation

Insights

Presents the pdf analysis as premium feature

PDF Analysis

Presents the zaia usage as premium feature

ZAIA

Global: Zendy Tools annual

Global: Zendy Free Plan

Global: Zendy Tools monthly

Global: Zendy Plus monthly

Weakly interacting massive particles are a widely well-probed dark mattercandidate by the dark matter direct detection experiments. Theoretically, thereare a large number of ultraviolet completed models that consist of a weaklyinteracting massive particle dark matter. The variety of models makes thecomparison with the direct detection data complicated and often non-trivial. Toovercome this, in the non-relativistic limit, the effective theory wasdeveloped in the literature which works very well to significantly reduce thecomplexity of dark matter-nucleon interactions and to better study the nuclearresponse functions. In the effective theory framework for a spin-1/2 darkmatter, we combine three independent likelihood functions from the latestPandaX, LUX, and XENON1T data, and give a joint limit on each effectivecoupling. The astrophysical uncertainties of the dark matter distribution arealso included in the likelihood. We further discuss the isospin violating casesof the interactions. Finally, for both dimension-five and dimension-sixeffective theories above the electroweak scale, we give updated limits of thenew physics mass scales.

A combined analysis of PandaX, LUX, and XENON1T experiments within the framework of dark matter effective theory